Non-equilibrium chemistry and cooling in the diffuse interstellar medium

A. J. Richings, J. Schaye and B. D. Oppenheimer


ISRF; nH, tot = 1 cm-3; Z = Zsol


Species log Tmin log Tmax log Tpeak Peak
CII 2.0 4.8 2.0 61.8 %
NII 2.0 4.3 2.0 13.4 %
SiII 2.0 4.0 2.7 42.4 %
FeII 2.4 4.0 3.7 23.9 %
SIII 2.5 4.1 3.7 14.1 %
SII 3.8 4.2 4.0 9.2 %
MgII 4.0 4.3 4.1 8.6 %
OII 3.8 4.8 4.1 31.2 %
HI 4.1 4.8 4.4 47.8 %
SiIII 4.3 4.8 4.6 11.0 %
CIII 4.5 5.1 4.8 31.7 %
HeII 4.7 5.2 4.9 19.0 %
OIII 4.7 5.3 5.0 20.5 %
CIV 4.9 5.2 5.1 14.1 %
NIV 5.1 5.3 5.2 10.1 %
OIV 5.0 5.5 5.2 41.1 %
OV 5.2 5.6 5.4 48.6 %
OVI 5.4 5.7 5.5 23.5 %
NeV 5.3 5.7 5.5 14.2 %
NeVI 5.5 5.8 5.6 30.8 %
MgVI 5.6 5.7 5.7 5.7 %
NeVII 5.6 5.9 5.7 16.8 %
FeVIII 5.6 6.0 5.8 10.9 %
MgVII 5.7 5.9 5.8 8.0 %
NeVIII 5.8 5.9 5.8 8.1 %
FeIX 5.7 6.2 5.9 30.6 %
MgVIII 5.8 6.0 5.9 11.3 %
SiVIII 5.9 6.1 6.0 6.0 %
FeX 5.9 6.2 6.1 21.0 %
SiIX 6.0 6.2 6.1 9.1 %
FeXII 6.1 6.3 6.2 11.4 %
SiX 6.1 6.2 6.2 7.4 %
FeXIII 6.1 6.4 6.2 18.2 %
SiXI 6.2 6.3 6.2 5.6 %
FeXIV 6.2 6.5 6.3 16.1 %
OVII 6.2 6.5 6.4 8.2 %
FeXV 6.2 6.7 6.4 19.1 %
OVIII 6.4 7.0 6.6 11.3 %
FeXVI 6.3 6.9 6.6 25.6 %
FeXVII 6.6 6.9 6.8 10.8 %
FeXVIII 6.8 7.0 6.9 9.1 %
FeXIX 6.9 7.1 7.0 7.4 %
FeXX 7.0 7.1 7.0 7.2 %
FeXXI 7.0 7.2 7.1 7.3 %
FeXXII 7.1 7.3 7.2 9.4 %
FeXXIII 7.1 7.4 7.3 9.0 %
FeXXIV 7.3 7.6 7.4 7.2 %
FeXXV 7.6 8.0 7.8 6.6 %
HeIII 6.6 9.0 8.9 27.6 %
HII 2.0 9.0 9.0 65.0 %


Last modified: Fri Mar 21 15:32:29 2014
Email: richings@strw.leidenuniv.nl